The ringing of quantum corrected Schwarzschild black hole with GUP

被引：6
作者：
Xing, Yujia [1 ]
Yang, Yi [1 ]
Liu, Dong [1 ]
Long, Zheng-Wen [1 ]
Xu, Zhaoyi [1 ]
机构：
[1] Guizhou Univ, Coll Phys, Guiyang 550025, Peoples R China
来源：
COMMUNICATIONS IN THEORETICAL PHYSICS | 2022年 / 74卷 / 08期
基金：
中国国家自然科学基金;
关键词：
quantum corrections; black hole; quasinormal mode; generalized uncertainty principle; LATE-TIME BEHAVIOR; NORMAL-MODES; STELLAR COLLAPSE; WKB APPROACH; EXPLOSIONS;
D O I：
10.1088/1572-9494/ac7cdc
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
Schwarzschild black holes with quantum corrections are studied under scalar field perturbations and electromagnetic field perturbations to analyze the effect of the correction term on the potential function and quasinormal mode (QNM). In classical general relativity, spacetime is continuous and there is no existence of the so-called minimal length. The introduction of the correction items of the generalized uncertainty principle, the parameter beta, can change the singularity structure of the black hole gauge and may lead to discretization in time and space. We apply the sixth-order WKB method to approximate the QNM of Schwarzschild black holes with quantum corrections and perform numerical analysis to derive the results of the method. Also, we find that the effective potential and QNM in scalar fields are larger than those in electromagnetic fields.
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页数：9
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